Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

Small but Plentiful: How the Faintest Galaxies Illuminated the Early Universe

09.07.2014

Light from tiny galaxies more than 13 billion years ago played a larger role than previously thought in creating the conditions in the universe as we know it today, according to a new study by researchers at the Georgia Institute of Technology and the San Diego Supercomputer Center (SDSC) at the University of California, San Diego.

Ultraviolet (UV) light from stars in these faint dwarf galaxies helped strip interstellar hydrogen of electrons in a process called reionization, researchers said in a paper published this week in the journal Monthly Notices of the Royal Astronomical Society. The epoch of reionization began about 200 million years after the Big Bang and astrophysicists agree that it took about 800 million more years for the entire universe to become reionized. It marked the last major phase transition of gas in the universe, and it remains ionized today.


A view of the entire simulation volume that shows the large scale structure of the gas distribution in filaments and clumps. The red regions are heated by stellar UV light coming from the galaxies, highlighted in white. These galaxies are over 1000 times less massive than the Milky Way and contributed nearly one-third of the UV light during reionization. The field of view of this image is 400,000 light years across, when the universe was only 700 million years old. John Wise, Georgia Institute of Technology.

Astrophysicists aren’t in agreement when it comes to determining which type of galaxies played major roles in this epoch. Most have focused on larger, more luminous galaxies. However, this latest research, based on computer simulations, indicates scientists should also focus on the smallest ones. Specifically, these new simulations show that these tiny galaxies – despite being 1000 times smaller in mass and 30 times smaller in size than the Milky Way – contributed nearly 30 percent of the UV light during this process.

Reionization experts often ignored these dwarf galaxies because they didn’t think they formed stars. It was assumed that UV light from nearby galaxies was too strong and suppressed these tiny neighbors.

“It turns out they did form stars, usually in one burst, around 500 million years after the Big Bang,” said John H. Wise, a Georgia Tech assistant professor in the School of Physics who led the study. “The galaxies were small, but so plentiful that they contributed a significant fraction of UV light in the reionization process.”

The team’s simulations modeled the flow of UV stellar light through the gas within galaxies as they formed. They found that the fraction of ionizing photons escaping into intergalactic space was 50 percent in small (more than 10 million solar masses) halos, or spheroidal collections of dark matter which is the site of galaxy formation. It was only 5 percent in larger halos (300 million solar masses).  This elevated fraction, combined with their high abundance, is exactly the reason why the faintest galaxies play an integral role during reionization.

“It’s very hard for UV light to escape galaxies because of the dense gas that fills them,” said Wise. “In small galaxies, there’s less gas between stars, making it easier for UV light to escape because it isn’t absorbed as quickly. Plus, supernova explosions can open up channels more easily in these tiny galaxies in which UV light can escape.”

The team’s simulation results provide a gradual timeline that tracks the progress of reionization over hundreds of millions of years. About 300 million years after the Big Bang, the universe was 20 percent ionized. It was 50 percent at 550 million years. The universe was fully ionized at 860 million years after its creation.

“That such small galaxies could contribute so much to reionization is a real surprise,” said Michael Norman, distinguished professor of physics at UC San Diego and one of the co-authors of the paper.

“Once again, the supercomputer is teaching us something new and unexpected, something that will need to be factored into future studies of reionization,” said Norman, who also is the director of SDSC, an Organized Research Unit of UC San Diego.

The term ‘reionized’ is used because the universe was ionized immediately after the fiery Big Bang. During that time, ordinary matter consisted mostly of hydrogen atoms with positively charged protons stripped of their negatively charged electrons. Eventually, the universe cooled enough for electrons and protons to combine and form neutral hydrogen. They didn’t give off any optical or UV light. Without the light, astrophysicists aren’t able to see traces of how the cosmos evolved during these Dark Ages using conventional telescopes. The light returned when reionization began, allowing experts such as Wise to pinpoint the youngest galaxies and study their features.

The research team expects to learn more about these faint galaxies when the next generation of telescopes is operational. For example, NASA’s James Webb Space Telescope, scheduled to launch in 2018, will be able to see them.

In addition to Wise and Norman, the research team included Vasiliy G. Demchenko and

Martin T. Halicek (Center for Relativistic Astrophysics, Georgia Institute of Technology); Matthew J. Turk (Department of Astronomy, Columbia University); Tom Abel (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University); and Britton D. Smith (Institute of Astronomy, University of Edinburgh). The research was supported by the National Science Foundation (NSF) under award numbers AST 1211626, AST 1333360, and AST 1109243.

Media Contact

Jan Zverina
858-534-5111
jzverina@sdsc.edu

Jan Zverina | Eurek Alert!
Further information:
http://ucsdnews.ucsd.edu/pressrelease/small_but_plentiful_how_the_faintest_galaxies_illuminated_the_early_univers

Further reports about: Astrophysics Big Bang Dwarf galaxies Universe dark matter dwarf electrons galaxies protons telescopes

More articles from Physics and Astronomy:

nachricht Tiny Drops of Early Universe 'Perfect' Fluid
02.09.2015 | Brookhaven National Laboratory

nachricht Cosmic recycling
02.09.2015 | European Southern Observatory ESO

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: How wind sculpted Earth's largest dust deposit

China's Loess Plateau was formed by wind alternately depositing dust or removing dust over the last 2.6 million years, according to a new report from University of Arizona geoscientists. The study is the first to explain how the steep-fronted plateau formed.

China's Loess Plateau was formed by wind alternately depositing dust or removing dust over the last 2.6 million years, according to a new report from...

Im Focus: An engineered surface unsticks sticky water droplets

The leaves of the lotus flower, and other natural surfaces that repel water and dirt, have been the model for many types of engineered liquid-repelling surfaces. As slippery as these surfaces are, however, tiny water droplets still stick to them. Now, Penn State researchers have developed nano/micro-textured, highly slippery surfaces able to outperform these naturally inspired coatings, particularly when the water is a vapor or tiny droplets.

Enhancing the mobility of liquid droplets on rough surfaces could improve condensation heat transfer for power-plant heat exchangers, create more efficient...

Im Focus: Increasingly severe disturbances weaken world's temperate forests

Longer, more severe, and hotter droughts and a myriad of other threats, including diseases and more extensive and severe wildfires, are threatening to transform some of the world's temperate forests, a new study published in Science has found. Without informed management, some forests could convert to shrublands or grasslands within the coming decades.

"While we have been trying to manage for resilience of 20th century conditions, we realize now that we must prepare for transformations and attempt to ease...

Im Focus: OU astrophysicist and collaborators find supermassive black holes in quasar nearest Earth

A University of Oklahoma astrophysicist and his Chinese collaborator have found two supermassive black holes in Markarian 231, the nearest quasar to Earth, using observations from NASA's Hubble Space Telescope.

The discovery of two supermassive black holes--one larger one and a second, smaller one--are evidence of a binary black hole and suggests that supermassive...

Im Focus: What would a tsunami in the Mediterranean look like?

A team of European researchers have developed a model to simulate the impact of tsunamis generated by earthquakes and applied it to the Eastern Mediterranean. The results show how tsunami waves could hit and inundate coastal areas in southern Italy and Greece. The study is published today (27 August) in Ocean Science, an open access journal of the European Geosciences Union (EGU).

Though not as frequent as in the Pacific and Indian oceans, tsunamis also occur in the Mediterranean, mainly due to earthquakes generated when the African...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

Networking conference in Heidelberg for outstanding mathematicians and computer scientists

20.08.2015 | Event News

Scientists meet in Münster for the world’s largest Chitin und Chitosan Conference

20.08.2015 | Event News

Large agribusiness management strategies

19.08.2015 | Event News

 
Latest News

Tiny Drops of Early Universe 'Perfect' Fluid

02.09.2015 | Physics and Astronomy

Learning from Nature: Genomic database standard alleviates search for novel antibiotics

02.09.2015 | Life Sciences

International research project gets high level of funding

02.09.2015 | Awards Funding

VideoLinks
B2B-VideoLinks
More VideoLinks >>>